Dissociative recombination of nitrile ions:: DCCCN+ and DCCCND+

被引:39
作者
Geppert, WD
Ehlerding, A
Hellberg, F
Semaniak, J
Österdahl, F
Kaminska, M
Al-Khalili, A
Zhaunerchyk, V
Thomas, R
Af Ugglas, M
Källberg, A
Simonsson, A
Larsson, M
机构
[1] Univ Stockholm, Dept Phys, SE-10691 Stockholm, Sweden
[2] Jan Kochanowski Univ Humanities & Sci, Inst Phys, PL-25406 Kielce, Poland
[3] Royal Inst Technol, Dept Phys, SE-10691 Stockholm, Sweden
[4] Manne Siegbahn Lab, SE-10405 Stockholm, Sweden
关键词
astrochemistry; methods : laboratory; molecular data;
D O I
10.1086/422335
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Branching ratios and absolute cross sections have been measured for the dissociative recombination of DCCCN+ and DCCCND+ using the CRYRING ion storage ring. In the case of DCCCN+ the dissociation yielding D + C3N and those leading to two fragments containing a pair of heavy atoms dominate, whereas pathways producing a fragment with three heavy atoms play only a minor role. Conversely, for DCCCND+, only those channels preserving the carbon chain or producing two fragments with a pair of heavy atoms each are detected. The cross sections of the reactions are very similar and can be fitted to the expressions sigma = (2.9 +/- 0.5) x 10(-15)E(eV)(-1.05 +/- 0.02) cm(2) and sigma = (2.3 +/- 0.4) x 10(-15)E(eV)(-1.10 +/- 0.02) cm(2) for DCCCN+ and DCCCND+, respectively. From these data, thermal reaction rates of k(T) = (1.5 +/- 0.3) x 10(-6)(T/300 K)(-0.60 +/- 0.02) cm(3) s(-1) and k(T) = (1.5 +/- 0.3) x 10(-6)(T/300 K)(-0.58 +/- 0.02) cm(3) s(-1) were calculated for DCCCN+ and DCCCND+, respectively. These rates and branching ratios are compared with those hitherto used in astrophysical models.
引用
收藏
页码:1302 / 1309
页数:8
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